Dynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12
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Coadvisor
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Undergraduate course
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Springer
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Article
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Acesso restrito
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Abstract
This paper considers the dynamics of two planets, as the planets B and C of the pulsar PSR B1257+12, near a 3/2 mean-motion resonance. A two-degrees-of-freedom model, in the framework of the general three-body planar problem, is used and the solutions are analyzed through surfaces of section and Fourier techniques in the full phase space of the system.
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Keywords
chaos, extra-solar planets, planetary systems, pulsar planets, resonance
Language
English
Citation
Celestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 94, n. 4, p. 381-397, 2006.
